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SWI_SPECTRAL_SCAN_CTS_PS_V1
SWI SPECTRAL SCAN CTS PS V1
Investigation of the atmospheric composition of Jupiter and the Galilean
moons. The whole frequency range available to SWI is scanned. This mode is nominally meant for deep integrations and requires numerous repetitions (e.g. monitoring of the moons). Two
CTS spectra are recorded for 60 seconds over 10000 channels (16bit coding). Position-switch
calibration method. A single execution can cover up to 13 tunings.

Pointing Type: S/C: nadir or limb. Instrument: nadir or limb, using the SWI mechanism if S/C points
nadir and to reach the moons
SWI

Pointing

nadir
-

Advanced

can be used from any JUICE-Jupiter distance, and from
anywhere for Galilean moons. Repetition: One full spectral scan for Jupiter in the equatorial
phase and another one in the high inclination phase (SWI LIMB SPECTRAL SCAN preferred),
one full spectral scan for all Galilean moons.
any rule that is used to schedule the observation: repetition rules, continuous (plasma instruments), one-off, every orbit, every day, etc
N/A
conditions that make the observation not possible (e.g. thruster firing)
#update2024Oct02

Commanding